Meteoric astronomy: A treatise on shooting-stars, fire-balls, and aerolites — John Shaqi
Meteoric astronomy: A treatise on shooting-stars, fire-balls, and aerolitesKirkwood, Daniel
Science
Meteoric astronomy: A treatise on shooting-stars, fire-balls, and aerolites
Kirkwood, Daniel
Meteors
It is well known that quantities of sand are often conveyed, by the
trade-winds, from the continent of Africa and deposited in the ocean.
Such sand-showers have sometimes occurred several hundred miles from
the coast. Volcanic matter also has been occasionally carried a
considerable distance. The phenomena above described cannot, however,
be referred to such causes; and there can be little doubt that most, if
not all of them, were of meteoric origin.
There is, in all probability, a regular gradation from the smallest
visible shooting-stars to bolides and aerolites. No doubt a great
number of very small meteoric stones penetrate beneath the earth's
surface and escape observation. An interesting account of the
accidental discovery of such _celestial pebbles_ has recently been
given by Professor Haidinger, of Vienna. The meteor from which they
were derived _was but little larger than an ordinary shooting-star_.
Its track was visible, however, until it terminated at the earth's
surface. Professor Haidinger's account is as follows: On the 31st
of July, 1859, about half-past nine o'clock in the evening, three
inhabitants of the bourg of Montpreis, in Styria, saw a small luminous
globe, very similar to a shooting-star, and followed by a luminous
streak in the heavens, fall directly to the earth, which it attained
close to the château that exists in the locality. The fall was
accompanied by a whistling or hissing noise in the air, and terminated
by a _slight_ detonation. The three observers, rushing to the spot
where the meteor fell, immediately found a small cavity in the hard,
sandy soil, from which they extracted three small meteoric stones about
the size of nuts, and a quantity of black powder. For five to eight
seconds these stones continued in a _state of incandescence_, and it
was necessary to allow upwards of a quarter of an hour to elapse before
they could be touched without inflicting a burn. They appear to have
been ordinary meteoric stones, covered with the usual black rind. The
possessors would not give them up to be analyzed. The details of this
remarkable occurrence of the fall of an extremely small meteor, we owe
to Herr Deschann, Conservator of the Museum of Laibach, in Carniola,
and member of the Austrian Chamber of Deputies.
Public-domain text, read in full here on John Shaqi.
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